3D self-consistent continuum radiative transfer code based on the Monte-Carlo Method
3D self-consistent N-body barred models of the Milky Way: I. Stellar dynamics
3D self-consistent N-body barred models of the Milky Way: II. Gas dynamics
3D Semiconductor Detectors For New Focusing Hard X And Soft Gamma-ray Telescopes
3D Simulation of Convection and Spectral Line Formation in A-type Stars
3D simulation of flux emergence from convective zone to corona with BATSRUS
3D Simulation of the Gas Dynamics in the Central Parsec of the Galaxy
3D simulations identifying the effects of varying the twist and field strength of an emerging flux tube
3D Simulations of Betelgeuse's Bow Shock
3D simulations of Einstein's equations: symmetric hyperbolicity, live gauges and dynamic control of the constraints
3D Simulations of Fluctuation Spectra in the Hall-MHD Plasma
3D Simulations of Galactic Winds in Dwarf Galaxies
3D simulations of gyrosynchrotron emission from mildly anisotropic nonuniform electron distributions in symmetric magnetic loops
3D simulations of linearized scalar fields in Kerr spacetime
3D simulations of M star atmosphere velocities and their influence on molecular FeH lines
3D Simulations of Magnetic Massive Star Winds
3D Simulations of Magnetohydrodynamic Waves in the Magnetized Solar Atmosphere
3D Simulations of MHD Jet Propagation Through Uniform and Stratified External Environments
3D simulations of microquasar jets in clumpy stellar winds
3D simulations of pillars formation around HII regions: the importance of shock curvature